Pankaj S. Joshi0521871042, 9780521871044, 9780511378904
Physical phenomena in astrophysics and cosmology involve gravitational collapse in a fundamental way. The final fate of a massive star when it collapses under its own gravity at the end of its life cycle is one of the most important questions in gravitation theory and relativistic astrophysics, and is the foundation of black hole physics. General relativity predicts that continual gravitational collapse gives rise to a space-time singularity. Quantum gravity may take over in such regimes to resolve the classical space-time singularity. This book investigates these issues, and shows how the visible ultra-dense regions arise naturally and generically as an outcome of dynamical gravitational collapse. It will be of interest to graduate students and academic researchers in gravitation physics, fundamental physics, astrophysics, and cosmology. It includes a detailed review of recent research into gravitational collapse, and several examples of collapse models are investigated in detail. |
Table of contents : Title
……Page 1 Contents
……Page 7 1. Introduction
……Page 11 2. The spacetime manifold
……Page 20 3. Spherical collapse
……Page 70 4. Cosmic censorship
……Page 145 5. Final fate of a massive star
……Page 220 References
……Page 265 Index
……Page 279 |
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